Search Publications

Ancient stellar populations in the outskirts of nearby grand-design spirals: Investigation of their star formation histories
DOI: 10.1051/0004-6361/202347626 Bibcode: 2024A&A...686A.124L

Bisigello, Laura; Renzini, Alvio; Rodighiero, Giulia +7 more

Context. The main sequence (MS) of star-forming galaxies (SFGs) is the tight relation between the galaxy stellar mass (M) and its star formation rate (SFR) and was observed up to z ∼ 6. The MS relation can be used as a reference for understanding the differences among galaxies, which are characterised by different rates of stellar prod…

2024 Astronomy and Astrophysics
Herschel 3
Atmospheric Characterization of the Super-Jupiter HIP 99770 b with KPIC
DOI: 10.3847/1538-3881/ad6609 Bibcode: 2024AJ....168..131Z

Zhang, Yapeng; Do Ó, Clarissa R.; Fitzgerald, Michael P. +28 more

Young, self-luminous super-Jovian companions discovered by direct imaging provide a challenging test for planet formation and evolution theories. By spectroscopically characterizing the atmospheric compositions of these super-Jupiters, we can constrain their formation histories. Here we present studies of the recently discovered HIP 99770 b, a 16 …

2024 The Astronomical Journal
Gaia 3
Curves of growth for transiting exocomets: Application to Fe II lines in the β Pictoris system
DOI: 10.1051/0004-6361/202347588 Bibcode: 2024A&A...684A.210V

Lecavelier des Etangs, A.; Vidal-Madjar, A.; Vrignaud, T. +4 more

Using transit spectroscopy, exocomets are routinely observed in the young planetary system of β Pic. However, despite more than 35 yr of observations, we still have very little information on the physical properties and almost no information on the abundances of the gaseous clouds surrounding the comets' nuclei, the difficulty being the conversion…

2024 Astronomy and Astrophysics
eHST 3
Radio Emission from High-redshift Active Galactic Nuclei in the JADES and CEERS Surveys
DOI: 10.3847/1538-3881/ad3b97 Bibcode: 2024AJ....167..251L

Whalen, Daniel J.; Latif, Muhammad A.; Aftab, Ammara

Recent calculations indicate that radio emission from quasars at z ∼ 6–7 could be detected at much earlier stages of evolution, at z ∼ 14–15, by the Next-Generation Very Large Array (ngVLA) and the Square Kilometer Array (SKA). However, the James Webb Space Telescope has now discovered less luminous active galactic nuclei (AGNs) at z > 4 and a …

2024 The Astronomical Journal
JWST 3
Passing Stars as an Important Driver of Paleoclimate and the Solar System's Orbital Evolution
DOI: 10.3847/2041-8213/ad24fb Bibcode: 2024ApJ...962L..28K

Raymond, Sean N.; Kaib, Nathan A.

Reconstructions of the paleoclimate indicate that ancient climatic fluctuations on Earth are often correlated with variations in its orbital elements. However, the chaos inherent in the solar system's orbital evolution prevents numerical simulations from confidently predicting Earth's past orbital evolution beyond 50–100 Myr. Gravitational interac…

2024 The Astrophysical Journal
Gaia 3
Searching for GEMS: TOI-6383Ab, a Giant Planet Transiting an M3-dwarf Star in a Binary System
DOI: 10.3847/1538-3881/ad7fe8 Bibcode: 2024AJ....168..273B

Kobulnicky, Henry A.; Cochran, William D.; Mahadevan, Suvrath +22 more

We report on the discovery of a transiting giant planet around the 3500 K M3-dwarf star TOI-6383A located 172 pc from Earth. It was detected by the Transiting Exoplanet Survey Satellite and confirmed by a combination of ground-based follow-up photometry and precise radial velocity measurements. This planet has an orbital period of ∼1.791 days, a m…

2024 The Astronomical Journal
Gaia 3
An in-depth analysis of the variable cyclotron lines in GX 301−2
DOI: 10.1051/0004-6361/202348841 Bibcode: 2024A&A...686A..95Z

Fürst, Felix; Kretschmar, Peter; Pottschmidt, Katja +13 more

Context. The high-mass X-ray binary system GX 301−2 is a persistent source with a well-known variable cyclotron line centered at 35 keV. Recently, a second cyclotron line at 50 keV has been reported with a presumably different behavior than the 35 keV line.
Aims: We investigate the presence of the newly discovered cyclotron line in the phase-…

2024 Astronomy and Astrophysics
Gaia 3
Galaxies in the zone of avoidance: Misclassifications using machine learning tools
DOI: 10.1051/0004-6361/202348637 Bibcode: 2024A&A...686A..18M

Minniti, D.; Masetti, N.; Soto, M. +10 more

Context. Automated methods for classifying extragalactic objects in large surveys offer significant advantages compared to manual approaches in terms of efficiency and consistency. However, the existence of the Galactic disk raises additional concerns. These regions are known for high levels of interstellar extinction, star crowding, and limited d…

2024 Astronomy and Astrophysics
Gaia XMM-Newton 3
Deciphering Radio Emissions from Accretion Disk Winds in Radio-quiet Active Galactic Nuclei
DOI: 10.3847/1538-4357/ad3a63 Bibcode: 2024ApJ...968..116Y

Inoue, Yoshiyuki; Yamada, Tomoya; Sakai, Nobuyuki +1 more

Unraveling the origins of radio emissions from radio-quiet active galactic nuclei (RQ AGNs) remains a pivotal challenge in astrophysics. One potential source of this radiation is the shock interaction between AGN disk winds and the interstellar medium (ISM). To understand this phenomenon, we construct a spherical, one-zone, and self-similar expans…

2024 The Astrophysical Journal
Herschel 3
Diagnosing the Particle Transport Mechanism in the Pulsar Halo via X-Ray Observations
DOI: 10.3847/1538-4357/ad43e1 Bibcode: 2024ApJ...969....9W

Liu, Ruo-Yu; Ge, Chong; Wu, Qi-Zuo +2 more

Pulsar halos (also termed "TeV halos") are a new class of γ-ray sources in the Galaxy, which manifest as extended γ-ray emission around middle-aged pulsars, as discovered around the Geminga pulsar, the Monogem pulsar, and PSR J0622+3749 by the High-Altitude Water Cherenkov Observatory and the Large High-Altitude Air Shower Observatory. A consensus…

2024 The Astrophysical Journal
XMM-Newton 3